{
  "annotation_id": "a3b14c74-d353-402f-90ed-2cb3d60b1ae3",
  "date_created": "2026-03-02T18:02:09.941000Z",
  "date_modified": "2026-03-02T18:02:09.941000Z",
  "file_hash": "59ab7850a928d1361b199ccd50caa5a6755ff68497e1c3375b80326af0fa03d5",
  "private": false,
  "record": {
    "abstract": "This paper examines how black holes might compute in light of recent models\nof the black-hole final state. These models suggest that quantum information\ncan escape from the black hole by a process akin to teleportation. They require\na specific final state and restrictions on the interaction between the\ncollapsing matter and the incoming Hawking radiation for quantum information to\nescape. This paper shows that for an arbitrary final state and for generic\ninteractions between matter and Hawking radiation, the quantum information\nabout how the hole was formed and the results of any computation performed by\nthe matter inside the hole escapes with fidelity exponentially close to 1.",
    "arxiv_id": "quant-ph/0406205",
    "authors": [
      "Seth Lloyd"
    ],
    "categories": [
      "quant-ph"
    ],
    "doi": "10.1103/PhysRevLett.96.061302",
    "journal_ref": "Phys.Rev.Lett. 96 (2006) 061302",
    "title": "Almost Certain Escape from Black Holes",
    "url": "https://arxiv.org/abs/quant-ph/0406205"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "73f8f22a-87cb-46a1-9c23-74ee6ba917b4",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}